Tests 2-3
Sirius
B is white.
Sirius
B is small but heavy.
[YES] to these two:
Sirius B is a White Dwarf. It is a star roughly the size of the Earth, but with roughly the mass of the Sun. Here is what the Harvard Bright Star Catalog (available from CDS as a Gzipped file, requiring Gunzip) has to say: "B is first white dwarf ever discovered; predicted by Bessel (1844) on basis of orbital motion of Sirius, it was first seen by Alvan Clark in 1862, and its peculiar high temperature, small size and great density established by W. Adams in 1925." (<-- First photo of Sirius A & B by Irving Lindenblad 1973) |
The first man to properly understand white dwarves was (Nobel laureate and died only in 1995) Subramanyan Chandrasekhar in 1928. Having a mass below what is now known as the Chandrasekhar Limit (1.4 solar masses), Sirius B avoided collapse into a Neutron Star or Black Hole; having used up its fuel, its gravitational collapse has been balanced by the exclusion principle of its so-called "degenerate electrons."
Our most recent numbers for the dimensions of Sirius B are presented in
Sirius B: A New, More Accurate View
by J.B. Holberg, M.A. Barstow, F.C. Bruhweiler, A.M. Cruise and A.J.
Penny
Astrophysical Journal v.497, p.935 04/1998 (Another great find
from NASA
ADS)
Temperature, mass (Mo), radius (Ro) take Holberg et al's figures without the ± margins for error. Data is from Extreme Ultraviolet Explorer (EUVE), and reprocessing of International Ultraviolet Explorer (IUE) data, and assuming the star is a perfect sphere.
Effective Temperature: (K) | 24,790 |
Mass: (Mo) | 1.034 |
Mass: (kg) | 2,056,626,000,000,000,000,000,000,000,000 |
Radius: (Ro) | 0.0084 |
Radius: (km) | 5838 |
Volume: (m3) | 833,452,553,034,495,433,745 |
Density: (kg/m3) | 2,467,598,176 |
Density: (tonne/cm3) | One heavy sugar cube at just less than 2.5 tonnes!!! |
Un Systeme Soudanais de Sirius presents this statement:
"It [Digitaria] is composed of a metal named sagala, a little brighter than iron, and of a weight that everyone on earth cannot lift it. The star weighs 480 mule loads (about 35,000 kg), or all grains, or all the iron on earth, if they were theoretically the size of a stretched cow hide or a mortar board." -- p287
In actual fact, 35 tonnes of Sirius B occupy only 14cm3. A mouse-hide perhaps...
Much more interesting is the Dogon concept of "Sagala," supposed to be shiny and metallic. It is a feat of tremendous imagination to name and give physical properties to white-dwarf material. Holberg and co. confirm that Sirius B is a "carbon core" white dwarf; it is known that white dwarfs start out hot and gradually cool to "black dwarfs". What is this matter chemically -- carbon-diamondoid? Can white-dwarf material separate from its "parent" and retain its integrity and structure? Could this be cool and stable? Could this be handled (if not picked up!)? Would it be reactive with normal matter, and if so how?
Anyone who could give sensible answers to these questions was
eligible for a prize
***The first prize falls***. Ralph Temple writes:
"If a bit of the material that composes Sirius B were to be removed from its parent star, assuming a feasible method, the mass thus removed would find itself separated from the gravity field that not only created it but must remain to make it stable, and the properties of normal matter would reassert themselves in short order. Probably violently. And with force that accelerated at a rate proportional to the square of the distance removed from the center of the gravity well." Thanks Ralph. So no keeping any sagala in my back yard then :-(
Test 4
Sirius
B has an orbit of 50 years.
[YES, BUT...] Sirius B does not in fact orbit around Sirius A.
The two stars orbit around a common centre of mass. We see an
apparent orbit.
The most recent number for this orbit P (Benest & Duvent 1995, see below) is 50.052 years.
Test 5
Sirius
B orbit is perpendicular to the horizon.
[NEARLY]
The angle of inclination i of Sirius B orbit is 136.62°
(Benest & Duvent 1995, see below)
Taking the Dogon statement to mean i = 180°, then
they are only 44° short (less than half a right angle).
Test 6
Sirius
B has rotational period of one year.
Considered unmeasurable by most ordinary mortals, Temperature,
Radius, and Rotational Velocity of Sirius B by Peter Thejll
and Harry L Shipman, Astronomical Society of the Pacific 98-922-926
(1986) [another paper from the NASA ADS]
claims to derive the interrelationships between radius,
rotational velocity and effective temperature for Sirius B, and
gives a range of possible equatorial velocities for Sirius B from
0 to 600 km/s. The Dogon are still in there; a period of rotation
of one year, based on Holberg et al's radius of 0.0084 Ro
(see above), gives an equatorial velocity of 0.00116 km/s.
In 1986, it appears that Sirius B numbers for temperature, mass,
radius, etc, were in doubt. Harvard Bright Star Catalog gives an
effective temperature of 32,000K; Thejll and Shipman date this to
1971. They themselves are working with a temperature of 26,000-28,000K
from IUE and Voyager 2 data. However, using Thejll and Shipman's
handy little diagram with Holberg's 1998 data (see above), a
rather different picture emerges.
So [NO] it would appear that the Period of Rotation of Sirius B
is less than a minute rather than a year.
Test 7
Sirius
B spins and ejects matter.
[YES] Sirius B spins. See Test 6 above. And
[YES] it ejects matter. From an overabundance of iron and
titanium in Sirius A's atmosphere, HBSC admits that there is a
"possibility that the atmosphere of Sirius A [is] polluted
by material ejected from Sirius B"
A and B are reported to be emitting soft (weak) X-rays so are
probably not exchanging matter as a cataclysmic variable, but
there must be gravitational interaction and tidal effects.
Picture shows a new, hot white dwarf star surrounded by the remnants of its red-giant shell. |
There may have been a closer connection in a previous stage of
stellar evolution, matching with the Chinese observation of a
"horn" on Sirius as described in the paper by Bonnet-Bidaud
and Gry in test 1.
In this artist's impression of a cataclysmic variable, mass flows as a distended ejecta looking uncannily like a placenta, a major feature of star formation described in Renard Pale. |
Test 8
Sirius
A scintillates at periastron and aposastron of Sirius B.
Any sensible answer to this strange assertion, unmatched by any
other culture or known observation will get a reward.
SCINTILLATION
Scintillation is the twinkling of stars (fluctuation of intensity)
seen through a planet's atmosphere. Scintillation in caused when
the star's light is distorted by the Earth's atmosphere.
Scintillation is greater for bright stars that are low on the
horizon. It is also known as astronomical scintillation. (ZoomSchool)
Test 9
Sirius B is remnant of first generation
star whose material formed others in the vicinity.
It is said that Sirius B age is about 1 Gyr. Any sensible
suggestions about how or not its matter may have formed nearby
stars is eligible for a prize.